Cylindrically Symmetric Solution in Teleparallel Theory of Gravitation

dc.creatorNashed, Gamal G. L.
dc.date2005-11-05
dc.date.accessioned2026-07-07T06:49:40Z
dc.date.available2026-07-07T06:49:40Z
dc.descriptionThe field equations of a special class of teleparallel theory of gravitation and electromagnetic fields have been applied to tetrad space having cylindrical symmetry with four unknown functions of radial coordinate $r$ and azimuth angle $θ$. The vacuum stress-energy momentum tensor with one assumption concerning its specific form generates one non-trivial exact analytic solution. This solution is characterized by a constant magnetic field parameter $B_0$. If $B_0=0$ then, the solution will reduces to the flat spacetime. The energy content is calculated using the superpotential given in the framework of teleparallel geometry. The energy contained in a sphere is found to be different from the pervious results.
dc.description12 pages, Latex
dc.identifierhttps://arxiv.org/abs/gr-qc/0511024
dc.identifierhttp://arxiv.org/abs/gr-qc/0511024
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/104434
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleCylindrically Symmetric Solution in Teleparallel Theory of Gravitation
dc.typetext

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